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- W2962730607 abstract "We discuss the early evolution of beryllium and oxygen in our Galaxy by comparing abundances of these elements for halo and disk metal-poor stars. Both, O and Be rise as we go progressively to more metal-rich stars, showing a slope 0.41 ± 0.09 ([Be/O] vs [Fe/H]) for stars with [Fe/H]≤ —1. This relationship provides an observational constraint to the actually proposed Galactic Cosmic Ray theories." @default.
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- W2962730607 date "2000-01-01" @default.
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- W2962730607 title "Galactic Evolution of Beryllium and Oxygen" @default.
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- W2962730607 doi "https://doi.org/10.1017/s0074180900166975" @default.
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